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Is the sulphur anomaly in planetary nebulae caused by the s-process?

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Shingles, Luke; Karakas, Amanda

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Motivated by unexplained observations of low sulphur abundances in planetary nebulae (PNe) and the PG1159 class of post-asymptotic giant branch (AGB) stars, we investigate the possibility that sulphur may be destroyed by nucleosynthetic processes in low-t

dc.contributor.authorShingles, Luke
dc.contributor.authorKarakas, Amanda
dc.date.accessioned2015-12-13T22:23:10Z
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/72629
dc.description.abstractMotivated by unexplained observations of low sulphur abundances in planetary nebulae (PNe) and the PG1159 class of post-asymptotic giant branch (AGB) stars, we investigate the possibility that sulphur may be destroyed by nucleosynthetic processes in low-t
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: ISM: Abundances; Nuclear reactions, nucleosynthesis, abundances; Planetary nebulae: general; Stars: AGB and post-AGB; Stars: evolution; Stars: Low-mass
dc.titleIs the sulphur anomaly in planetary nebulae caused by the s-process?
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume431
dc.date.issued2013
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB3348
local.type.statusPublished Version
local.contributor.affiliationShingles, Luke, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.description.embargo2037-12-31
local.bibliographicCitation.issue3
local.bibliographicCitation.startpage2861
local.bibliographicCitation.lastpage2871
local.identifier.doi10.1093/mnras/stt386
dc.date.updated2016-02-24T09:09:35Z
local.identifier.scopusID2-s2.0-84877025568
local.identifier.thomsonID000318347500071
CollectionsANU Research Publications

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